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High-Resolution Space-Weather Model,
15-9146
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Principal Investigators
Geoffrey Crowley
Christopher J. Freitas
Inclusive Dates: 07/01/99 - Current
Background - Space-weather refers to those
conditions on the sun, in the solar wind, magnetosphere, ionosphere, thermosphere, and
mesosphere, that can influence the performance and reliability of space-borne and
ground-based technological systems and can endanger human life or health. One goal of the
National Space Weather Program is to produce weather forecasts for the entire region of
space ranging from the sun to the Earth's middle atmosphere. Although existing simpler
models can simulate individual parts of the system, the goal of forecasting the entire
system is still several years away. Analogous with meteorology, various advances are
needed, including: increased speed of the models, models with higher resolution, data
assimilation, and the ability to forecast the inputs that drive the models. SwRI has
developed a parallelized model of the 30- to 500-kilometer altitude region including the
mesosphere, thermosphere, and ionosphere. In this research project, the team is seeking to
improve the performance and accuracy of the existing model.
Approach - The new model, based on the SwRI
parallelized Thermosphere-Ionosphere-Mesosphere-Electrodynamics (TIMEGCM) model, would
span the mesosphere, ionosphere, and thermosphere. The goal is to address performance
issues and model accuracy by implementing a Patched-Overset Grid capability based on the
existing model. In this approach, a base-grid is constructed using patched grid blocks, in
which the grid resolution in each block is uniform but potentially different from that in
adjacent blocks. Interpolation functions then define the relationship of flow parameters
across the patched interface of adjoining grid blocks. The dynamic variation of this
approach is called Overset Grids. A hierarchy of overlying grid systems dynamically moves
through the base grid and may have significantly finer grid resolutions than the base grid
system. A secondary goal of the proposed work is to improve the input specification to the
model by using the Assimilative Mapping of Ionospheric Electrodynamics (AMIE) technique to
provide realistic high-latitude inputs.
Accomplishments - The existing parallelized
TIMEGCM is being modified to accept high-latitude inputs specified by the AMIE technique.
Specifically this modification includes particle precipitation and electric potential
distribution throughout the high-latitude regions. The patched grid system for the new
version of TIMEGCM is being designed.
Space Sciences Program
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